The web of three-planet resonances in the outer Solar System

被引：46
|
作者：
Guzzo, M [1 ]
机构：
[1] Univ Padua, Dipartimento Matemat Pura & Applicata, I-35131 Padua, Italy
来源：
ICARUS | 2005年 / 174卷 / 01期
关键词：
planetary dynamics; Jovian planets; resonances; celestial mechanics;
D O I：
10.1016/j.icarus.2004.10.015
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper we numerically detect the web of three-planet resonances (i.e., resonances among mean anomalies, nodes and perihelia of three planets) with respect to the variation of the semi-major axis of Saturn and Jupiter, in a model including the planets from Jupiter to Neptune. The measure confirms the relevance of these resonances in the long-term evolution of the outer Solar System and provides a technique to identify some of the related coefficients. (c) 2004 Elsevier Inc. All rights reserved.
引用
收藏
页码：273 / 284
页数：12
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